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Searching for Low-Mass Supermassive Black Holes

Published online by Cambridge University Press:  25 May 2016

Michele Cappellari ,
Francesco Bertola ,
Enrico M. Corsini ,
José G. Funes S.J. ,
Alessandro Pizzella  and
Juan C. Vega Beltrán
Michele Cappellari
Affiliation:
Dipartimento di Astronomia, Università di Padova, Italy
Francesco Bertola
Affiliation:
Dipartimento di Astronomia, Università di Padova, Italy
Enrico M. Corsini
Affiliation:
Dipartimento di Astronomia, Università di Padova, Italy
José G. Funes S.J.
Affiliation:
Dipartimento di Astronomia, Università di Padova, Italy
Alessandro Pizzella
Affiliation:
European Southern Observatory, Santiago, Chile
Juan C. Vega Beltrán
Affiliation:
Osservatorio Astronomico di Padova, TNG, Italy

Extract

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It has become generally accepted that most or possibly all ellipticals and bulges of spirals harbor supermassive black holes in their center (see Ho 1998 for a recent review).

Type
IV. AGN Related Phenomena
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 422 - 423
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Bertola, F., Cappellari, M., Funes, J.G., Corsini, E.M., Pizzella, A., & Vega Beltrán, J.C. 1998, ApJL, in press [astro-ph/9807075] Google Scholar
Ho, L.C. 1998, in Observational Evidence for Black Hole in the Universe, ed. Chakrabati, S.K. (Dodrecht: Kluver Academic Publishers), in press [astro-ph/9803307] Google Scholar